Dynamics of the TrES-2 system

Details Dynamics of the TrES-2 system Dynamics of the TrES-2 system

2009-05-12

arxiv.org/abs/0905.1806v1

Astronomy and Astrophysics

Astrophysics

Earth and Planetary Astrophysics

accepted for publication in AN 330 (2009)

Scientific paper

The TrES-2 system harbors one planet which was discovered with the transit technique. In this work we investigate the dynamical behavior of possible additional, lower-mass planets. We identify the regions where such planets can move on stable orbits and show how they depend on the initial eccentricity and inclination. We find, that there are stable regions inside and outside the orbit of TrES-2b where additional, smaller planets can move. We also show that those planets can have a large orbital inclination which makes a detection with the transit technique very difficult.

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